Influence of Gauss-Bonnet Coupling Parameter on the Thermodynamic Properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet Black Holes
Abstract This paper deals in the thermodynamic properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet black holes. It exhibits the various stable and unstable phases of the black holes in these two modified gravity theories. In the first section, that reveals the various aspects of...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Chowdhury, Ratul [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2011 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media, LLC 2011 |
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| Übergeordnetes Werk: |
Enthalten in: International journal of theoretical physics - Springer US, 1968, 50(2011), 5 vom: 20. Jan., Seite 1628-1642 |
|---|---|
| Übergeordnetes Werk: |
volume:50 ; year:2011 ; number:5 ; day:20 ; month:01 ; pages:1628-1642 |
| Links: |
|---|
| DOI / URN: |
10.1007/s10773-011-0672-7 |
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| Katalog-ID: |
OLC2052375260 |
|---|
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| 520 | |a Abstract This paper deals in the thermodynamic properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet black holes. It exhibits the various stable and unstable phases of the black holes in these two modified gravity theories. In the first section, that reveals the various aspects of Einstein-Gauss-Bonnet black holes, we chose to study the changes in the Hawking Temperature with variations in the radius of event horizon (r) and charge (Q); and tried to justify them physically. Secondly in case of Einstein-Yang-Mills-Gauss-Bonnet black holes, we have attempted to compare the changes in the various thermodynamic parameters with varying r and Q; with the Einstein-Gauss-Bonnet black holes at a macroscopic level. Here we have considered the Yang Mills tensor, electromagnetic Lagrangian added to the action integrand. Again this very work deals in drawing out the similarities between these two types of black holes, thereby throwing some light on the aspect of black hole stability. Later we have also introspected the effects of the Gauss-Bonnet coupling parameter α, whose function (6αr), is added as a correction term to the black hole entropy. We have especially focused on what changes does it have upon the nature of the plots as to whether it enhances or reduces the effect of Q on the behavior of the curves. Finally this paper has also kept an eye at estimating the stability domains of the black holes described in these two gravity theories. | ||
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10.1007/s10773-011-0672-7 doi (DE-627)OLC2052375260 (DE-He213)s10773-011-0672-7-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Chowdhury, Ratul verfasserin aut Influence of Gauss-Bonnet Coupling Parameter on the Thermodynamic Properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet Black Holes 2011 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC 2011 Abstract This paper deals in the thermodynamic properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet black holes. It exhibits the various stable and unstable phases of the black holes in these two modified gravity theories. In the first section, that reveals the various aspects of Einstein-Gauss-Bonnet black holes, we chose to study the changes in the Hawking Temperature with variations in the radius of event horizon (r) and charge (Q); and tried to justify them physically. Secondly in case of Einstein-Yang-Mills-Gauss-Bonnet black holes, we have attempted to compare the changes in the various thermodynamic parameters with varying r and Q; with the Einstein-Gauss-Bonnet black holes at a macroscopic level. Here we have considered the Yang Mills tensor, electromagnetic Lagrangian added to the action integrand. Again this very work deals in drawing out the similarities between these two types of black holes, thereby throwing some light on the aspect of black hole stability. Later we have also introspected the effects of the Gauss-Bonnet coupling parameter α, whose function (6αr), is added as a correction term to the black hole entropy. We have especially focused on what changes does it have upon the nature of the plots as to whether it enhances or reduces the effect of Q on the behavior of the curves. Finally this paper has also kept an eye at estimating the stability domains of the black holes described in these two gravity theories. Black hole thermodynamics Gauss-Bonnet gravity Black hole entropy Phase transition Biswas, Ritabrata aut Mazumder, Nairwita aut Chakraborty, Subenoy aut Enthalten in International journal of theoretical physics Springer US, 1968 50(2011), 5 vom: 20. Jan., Seite 1628-1642 (DE-627)129546097 (DE-600)218277-4 (DE-576)014996413 0020-7748 nnns volume:50 year:2011 number:5 day:20 month:01 pages:1628-1642 https://doi.org/10.1007/s10773-011-0672-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_24 GBV_ILN_70 GBV_ILN_2005 33.00 VZ AR 50 2011 5 20 01 1628-1642 |
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10.1007/s10773-011-0672-7 doi (DE-627)OLC2052375260 (DE-He213)s10773-011-0672-7-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Chowdhury, Ratul verfasserin aut Influence of Gauss-Bonnet Coupling Parameter on the Thermodynamic Properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet Black Holes 2011 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC 2011 Abstract This paper deals in the thermodynamic properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet black holes. It exhibits the various stable and unstable phases of the black holes in these two modified gravity theories. In the first section, that reveals the various aspects of Einstein-Gauss-Bonnet black holes, we chose to study the changes in the Hawking Temperature with variations in the radius of event horizon (r) and charge (Q); and tried to justify them physically. Secondly in case of Einstein-Yang-Mills-Gauss-Bonnet black holes, we have attempted to compare the changes in the various thermodynamic parameters with varying r and Q; with the Einstein-Gauss-Bonnet black holes at a macroscopic level. Here we have considered the Yang Mills tensor, electromagnetic Lagrangian added to the action integrand. Again this very work deals in drawing out the similarities between these two types of black holes, thereby throwing some light on the aspect of black hole stability. Later we have also introspected the effects of the Gauss-Bonnet coupling parameter α, whose function (6αr), is added as a correction term to the black hole entropy. We have especially focused on what changes does it have upon the nature of the plots as to whether it enhances or reduces the effect of Q on the behavior of the curves. Finally this paper has also kept an eye at estimating the stability domains of the black holes described in these two gravity theories. Black hole thermodynamics Gauss-Bonnet gravity Black hole entropy Phase transition Biswas, Ritabrata aut Mazumder, Nairwita aut Chakraborty, Subenoy aut Enthalten in International journal of theoretical physics Springer US, 1968 50(2011), 5 vom: 20. Jan., Seite 1628-1642 (DE-627)129546097 (DE-600)218277-4 (DE-576)014996413 0020-7748 nnns volume:50 year:2011 number:5 day:20 month:01 pages:1628-1642 https://doi.org/10.1007/s10773-011-0672-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_24 GBV_ILN_70 GBV_ILN_2005 33.00 VZ AR 50 2011 5 20 01 1628-1642 |
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10.1007/s10773-011-0672-7 doi (DE-627)OLC2052375260 (DE-He213)s10773-011-0672-7-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Chowdhury, Ratul verfasserin aut Influence of Gauss-Bonnet Coupling Parameter on the Thermodynamic Properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet Black Holes 2011 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC 2011 Abstract This paper deals in the thermodynamic properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet black holes. It exhibits the various stable and unstable phases of the black holes in these two modified gravity theories. In the first section, that reveals the various aspects of Einstein-Gauss-Bonnet black holes, we chose to study the changes in the Hawking Temperature with variations in the radius of event horizon (r) and charge (Q); and tried to justify them physically. Secondly in case of Einstein-Yang-Mills-Gauss-Bonnet black holes, we have attempted to compare the changes in the various thermodynamic parameters with varying r and Q; with the Einstein-Gauss-Bonnet black holes at a macroscopic level. Here we have considered the Yang Mills tensor, electromagnetic Lagrangian added to the action integrand. Again this very work deals in drawing out the similarities between these two types of black holes, thereby throwing some light on the aspect of black hole stability. Later we have also introspected the effects of the Gauss-Bonnet coupling parameter α, whose function (6αr), is added as a correction term to the black hole entropy. We have especially focused on what changes does it have upon the nature of the plots as to whether it enhances or reduces the effect of Q on the behavior of the curves. Finally this paper has also kept an eye at estimating the stability domains of the black holes described in these two gravity theories. Black hole thermodynamics Gauss-Bonnet gravity Black hole entropy Phase transition Biswas, Ritabrata aut Mazumder, Nairwita aut Chakraborty, Subenoy aut Enthalten in International journal of theoretical physics Springer US, 1968 50(2011), 5 vom: 20. Jan., Seite 1628-1642 (DE-627)129546097 (DE-600)218277-4 (DE-576)014996413 0020-7748 nnns volume:50 year:2011 number:5 day:20 month:01 pages:1628-1642 https://doi.org/10.1007/s10773-011-0672-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_24 GBV_ILN_70 GBV_ILN_2005 33.00 VZ AR 50 2011 5 20 01 1628-1642 |
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10.1007/s10773-011-0672-7 doi (DE-627)OLC2052375260 (DE-He213)s10773-011-0672-7-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Chowdhury, Ratul verfasserin aut Influence of Gauss-Bonnet Coupling Parameter on the Thermodynamic Properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet Black Holes 2011 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC 2011 Abstract This paper deals in the thermodynamic properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet black holes. It exhibits the various stable and unstable phases of the black holes in these two modified gravity theories. In the first section, that reveals the various aspects of Einstein-Gauss-Bonnet black holes, we chose to study the changes in the Hawking Temperature with variations in the radius of event horizon (r) and charge (Q); and tried to justify them physically. Secondly in case of Einstein-Yang-Mills-Gauss-Bonnet black holes, we have attempted to compare the changes in the various thermodynamic parameters with varying r and Q; with the Einstein-Gauss-Bonnet black holes at a macroscopic level. Here we have considered the Yang Mills tensor, electromagnetic Lagrangian added to the action integrand. Again this very work deals in drawing out the similarities between these two types of black holes, thereby throwing some light on the aspect of black hole stability. Later we have also introspected the effects of the Gauss-Bonnet coupling parameter α, whose function (6αr), is added as a correction term to the black hole entropy. We have especially focused on what changes does it have upon the nature of the plots as to whether it enhances or reduces the effect of Q on the behavior of the curves. Finally this paper has also kept an eye at estimating the stability domains of the black holes described in these two gravity theories. Black hole thermodynamics Gauss-Bonnet gravity Black hole entropy Phase transition Biswas, Ritabrata aut Mazumder, Nairwita aut Chakraborty, Subenoy aut Enthalten in International journal of theoretical physics Springer US, 1968 50(2011), 5 vom: 20. Jan., Seite 1628-1642 (DE-627)129546097 (DE-600)218277-4 (DE-576)014996413 0020-7748 nnns volume:50 year:2011 number:5 day:20 month:01 pages:1628-1642 https://doi.org/10.1007/s10773-011-0672-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_24 GBV_ILN_70 GBV_ILN_2005 33.00 VZ AR 50 2011 5 20 01 1628-1642 |
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10.1007/s10773-011-0672-7 doi (DE-627)OLC2052375260 (DE-He213)s10773-011-0672-7-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Chowdhury, Ratul verfasserin aut Influence of Gauss-Bonnet Coupling Parameter on the Thermodynamic Properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet Black Holes 2011 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC 2011 Abstract This paper deals in the thermodynamic properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet black holes. It exhibits the various stable and unstable phases of the black holes in these two modified gravity theories. In the first section, that reveals the various aspects of Einstein-Gauss-Bonnet black holes, we chose to study the changes in the Hawking Temperature with variations in the radius of event horizon (r) and charge (Q); and tried to justify them physically. Secondly in case of Einstein-Yang-Mills-Gauss-Bonnet black holes, we have attempted to compare the changes in the various thermodynamic parameters with varying r and Q; with the Einstein-Gauss-Bonnet black holes at a macroscopic level. Here we have considered the Yang Mills tensor, electromagnetic Lagrangian added to the action integrand. Again this very work deals in drawing out the similarities between these two types of black holes, thereby throwing some light on the aspect of black hole stability. Later we have also introspected the effects of the Gauss-Bonnet coupling parameter α, whose function (6αr), is added as a correction term to the black hole entropy. We have especially focused on what changes does it have upon the nature of the plots as to whether it enhances or reduces the effect of Q on the behavior of the curves. Finally this paper has also kept an eye at estimating the stability domains of the black holes described in these two gravity theories. Black hole thermodynamics Gauss-Bonnet gravity Black hole entropy Phase transition Biswas, Ritabrata aut Mazumder, Nairwita aut Chakraborty, Subenoy aut Enthalten in International journal of theoretical physics Springer US, 1968 50(2011), 5 vom: 20. Jan., Seite 1628-1642 (DE-627)129546097 (DE-600)218277-4 (DE-576)014996413 0020-7748 nnns volume:50 year:2011 number:5 day:20 month:01 pages:1628-1642 https://doi.org/10.1007/s10773-011-0672-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_24 GBV_ILN_70 GBV_ILN_2005 33.00 VZ AR 50 2011 5 20 01 1628-1642 |
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International journal of theoretical physics |
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Influence of Gauss-Bonnet Coupling Parameter on the Thermodynamic Properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet Black Holes |
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Influence of Gauss-Bonnet Coupling Parameter on the Thermodynamic Properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet Black Holes |
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Chowdhury, Ratul |
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International journal of theoretical physics |
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International journal of theoretical physics |
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2011 |
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Chowdhury, Ratul Biswas, Ritabrata Mazumder, Nairwita Chakraborty, Subenoy |
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10.1007/s10773-011-0672-7 |
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530 |
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influence of gauss-bonnet coupling parameter on the thermodynamic properties of einstein-gauss-bonnet and einstein-yang-mills-gauss-bonnet black holes |
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Influence of Gauss-Bonnet Coupling Parameter on the Thermodynamic Properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet Black Holes |
| abstract |
Abstract This paper deals in the thermodynamic properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet black holes. It exhibits the various stable and unstable phases of the black holes in these two modified gravity theories. In the first section, that reveals the various aspects of Einstein-Gauss-Bonnet black holes, we chose to study the changes in the Hawking Temperature with variations in the radius of event horizon (r) and charge (Q); and tried to justify them physically. Secondly in case of Einstein-Yang-Mills-Gauss-Bonnet black holes, we have attempted to compare the changes in the various thermodynamic parameters with varying r and Q; with the Einstein-Gauss-Bonnet black holes at a macroscopic level. Here we have considered the Yang Mills tensor, electromagnetic Lagrangian added to the action integrand. Again this very work deals in drawing out the similarities between these two types of black holes, thereby throwing some light on the aspect of black hole stability. Later we have also introspected the effects of the Gauss-Bonnet coupling parameter α, whose function (6αr), is added as a correction term to the black hole entropy. We have especially focused on what changes does it have upon the nature of the plots as to whether it enhances or reduces the effect of Q on the behavior of the curves. Finally this paper has also kept an eye at estimating the stability domains of the black holes described in these two gravity theories. © Springer Science+Business Media, LLC 2011 |
| abstractGer |
Abstract This paper deals in the thermodynamic properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet black holes. It exhibits the various stable and unstable phases of the black holes in these two modified gravity theories. In the first section, that reveals the various aspects of Einstein-Gauss-Bonnet black holes, we chose to study the changes in the Hawking Temperature with variations in the radius of event horizon (r) and charge (Q); and tried to justify them physically. Secondly in case of Einstein-Yang-Mills-Gauss-Bonnet black holes, we have attempted to compare the changes in the various thermodynamic parameters with varying r and Q; with the Einstein-Gauss-Bonnet black holes at a macroscopic level. Here we have considered the Yang Mills tensor, electromagnetic Lagrangian added to the action integrand. Again this very work deals in drawing out the similarities between these two types of black holes, thereby throwing some light on the aspect of black hole stability. Later we have also introspected the effects of the Gauss-Bonnet coupling parameter α, whose function (6αr), is added as a correction term to the black hole entropy. We have especially focused on what changes does it have upon the nature of the plots as to whether it enhances or reduces the effect of Q on the behavior of the curves. Finally this paper has also kept an eye at estimating the stability domains of the black holes described in these two gravity theories. © Springer Science+Business Media, LLC 2011 |
| abstract_unstemmed |
Abstract This paper deals in the thermodynamic properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet black holes. It exhibits the various stable and unstable phases of the black holes in these two modified gravity theories. In the first section, that reveals the various aspects of Einstein-Gauss-Bonnet black holes, we chose to study the changes in the Hawking Temperature with variations in the radius of event horizon (r) and charge (Q); and tried to justify them physically. Secondly in case of Einstein-Yang-Mills-Gauss-Bonnet black holes, we have attempted to compare the changes in the various thermodynamic parameters with varying r and Q; with the Einstein-Gauss-Bonnet black holes at a macroscopic level. Here we have considered the Yang Mills tensor, electromagnetic Lagrangian added to the action integrand. Again this very work deals in drawing out the similarities between these two types of black holes, thereby throwing some light on the aspect of black hole stability. Later we have also introspected the effects of the Gauss-Bonnet coupling parameter α, whose function (6αr), is added as a correction term to the black hole entropy. We have especially focused on what changes does it have upon the nature of the plots as to whether it enhances or reduces the effect of Q on the behavior of the curves. Finally this paper has also kept an eye at estimating the stability domains of the black holes described in these two gravity theories. © Springer Science+Business Media, LLC 2011 |
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Influence of Gauss-Bonnet Coupling Parameter on the Thermodynamic Properties of Einstein-Gauss-Bonnet and Einstein-Yang-Mills-Gauss-Bonnet Black Holes |
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Biswas, Ritabrata Mazumder, Nairwita Chakraborty, Subenoy |
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